When a White Dwarf takes on enough mass in this manner, it reaches a level called the chandrasekhar limit.
当一颗白矮星以这种方式增长到足够的质量时，它将达到钱德拉·塞卡极限。
It is then referred to as a White Dwarf.
这时，它被称为白矮星。
Volantis was overrun with White Dwarf elephants.
瓦兰提斯大街小巷到处都是白矮象。
This novel is like a White Dwarf, all mass and density.
这部小说像一个白矮星，通篇篇幅大却又缜密。
Or, it seems, when you're cruising past a White Dwarf star.
或者可以说在你缓慢驶过一颗白矮星时。
The primary target is a White Dwarf star known as GD358 in the constellation Hercules.
第一颗目标恒星是武仙星群中一颗称为GD358的白矮星。
The star, which was similar to our sun, had died peacefully and turned into a dense White Dwarf.
这颗和我们太阳类似的恒星，已经安然逝去并演变成了一颗密实的白矮星。
A White Dwarf retains about half of its mass but becomes incredibly dense because of its small size.
白矮星的质量只有以前的一半，体积很小，因此非常致密。
A White Dwarf is a "dead" star that doesn't generate its own energy like the sun does, Provencal says.
Provencal表示，白矮星是一颗“死”恒星，不像太阳那样自己生成能量。
The star was a White Dwarf called GD 362, and it's 150 light years from Earth, still within our galaxy.
GD 362是颗白矮星，距离地球150光年，也在银河系。
When a White Dwarf takes on enough mass in this manner it reaches a level called the chandrasekhar limit.
当一颗白矮星以这种方式增长到足够的质量时，它将达到一个称为钱德拉·塞卡极限的质量标准。
His team used observations from NASA's Spitzer space telescope to investigate dead White Dwarf stars.
他的队伍通过美国国家航空与宇宙航行局的施皮策望远镜去观察一些白矮星。
The hot, remnant stellar core of NGC 2818 will eventually cool off for billions of years as a White Dwarf.
炽热的恒星内核会在几十亿年里逐渐冷却，内核在这段时间里叫做白矮星。
In this model, gas flows from the large red giant companion star into a disk and then onto the White Dwarf.
这个模型是指气体从大型红巨星伴星流到白矮星的吸积盘上然后被吸进白矮星中。
Some day, millions of years from now, LS IV-14 116 will cool off to the point where it becomes a bona fide White Dwarf.
某天，几百万年后，LSIV - 14 116将会冷却形成真正的白矮星。
An astronomer makes the case that the best place to search for habitable planets may be very close to White Dwarf stars.
一位天文学家提出了一种新想法，在靠近白矮星的地方找最寻适合生命居住的行星。
The center of that star then transformed into a White Dwarf, at once very hot (more than 100, 000 Kelvin) and very small.
恒星的中心变成了白矮星，曾经非常热(10万k)非常小。
Researchers first observed accelerated expansion by studying Type Ia supernovae-the explosive deaths of White Dwarf stars.
研究人员在研究Ia型超新星——白矮星爆炸中的消亡过程时首度观察到加速的膨胀。
Our sun should become a White Dwarf in about five billion years. The process will destroy Mercury, Venus and possibly Earth.
太阳在50亿年后也将变成白矮星，届时将摧毁水星、金星甚至地球。
The tightly wound White Dwarf binary should also be radiating gravitational waves-ripples in the fabric of space and time.
紧紧缠绕的白矮双子星同时也会发出引力波——那是在空间和时间结构上扩散开的波纹。
The observations also show for the first time that a white dwarf can create a cavity around it before blowing up in a Type Ia event.
观测结果还首次显示，白矮星在爆炸成为Ia型超新星之前，会在其周围创造一个空洞。
Eventually—over tens or even hundreds of billions of years—a white dwarf cools until it becomes a black dwarf, which emits no energy.
在几百亿年甚至几千亿年之后，白矮星最终冷却形成黑矮星，后者不再散发任何能量。
It is also a circumbinary planet, orbiting around a binary system composed of the pulsar PSR B1620-26 a and the White Dwarf WD B1620-26.
Methuselah同时也是一颗circumbinary行星，它围绕着一个双星系统旋转，这个双星系统由脉冲星PS rB1620 - 26a和白矮星wd B1620 - 26组成。
If a binary includes a White Dwarf, gas pulled from a companion onto the White Dwarf's surface can fuse violently in a flash called a nova.
如果一个双星系统包含一个白矮星，从伴星上抽离的气体会落在白矮星的表面，在一瞬间引发猛烈的聚变反应，即新星。
The team found the dancing stars while surveying for White Dwarf pairs using the 6.5-meter Multiple Mirror Telescope on Arizona's Mount Hopkins.
这支研究团队是在观测白矮星对时发现这对翩翩起舞的双星的，当时他们使用的是位于亚利桑那州霍普金斯山上的多镜望远镜。
At that speed, HM Cancri is the fastest binary star pair ever discovered, with each White Dwarf circling the other at a speed of 310 miles per second.
双星HMCancri是迄今为止所发现的运行最快的双星，它们是一对白矮星，其中一个围绕着另一个运转的速度是每秒310英里。
This leads the researchers to suspect that a white dwarf star strayed too close to the intermediate-mass black hole and was ripped apart by tidal forces.
这导致研究人员怀疑一个迷途的白矮星离某个中等质量黑洞太接近了，并受其潮汐引力的撕扯。
This leads the researchers to suspect that a white dwarf star strayed too close to the intermediate-mass black hole and was ripped apart by tidal forces.
这导致研究人员怀疑一个迷途的白矮星离某个中等质量黑洞太接近了，并受其潮汐引力的撕扯。
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